Data on Stark Broadening of N VI Spectral Lines

Milan S. Dimitrijević; Magdalena D. Christova; Sylvie Sahal-Bréchot

doi:10.20944/preprints202403.1366.v1

Preprint Data Descriptor Version 1 Preserved in Portico This version is not peer-reviewed

Version 1 : Received: 21 March 2024 / Approved: 22 March 2024 / Online: 22 March 2024 (11:45:43 CET)

Data on Stark broadening parameters, spectral line widths and shifts, for 15 multiplets of N VI, which spectral lines are broadened by collisions with electrons, protons, alpha particles (He III) and B III, B IV, B V and B VI ions, are presented. They have been calculated, using the semiclassical perturbation theory, for temperatures from 50,000 K to 2,000,000 K, and perturber densities from 1016 cm−3 up to 1024 cm−3. These data are particularly of interest for the analysis and modelling of atmospheres of hot and dense stars, as e.g. white dwarfs, and for investigation of their spectra, but also for analyis ad modelling of laser driven plasma in proton-boron fusion research.

atomic data; Stark broadening; N VI; proton-boron fusion; line profiles; atomic processes; stellar atmospheres

Physical Sciences, Atomic and Molecular Physics

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Data on Stark Broadening of N VI Spectral Lines

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